Table 2: Minimum distance from the plane of Sgr A*, $\vert z\vert _{\rm min}$, vs. projected radius r for five stars with $R_{\rm min} > r$. The values are based on 2.58$\sigma $ (99% confidence level) acceleration upper limits. Only stars with r<0.024 pc are sufficiently constrained; see Fig. 19.
Star ID r [mpc] $\vert z\vert _{\rm min}$ [mpc]
823 19.2 12.9
832 23.2 8.6
1333 20.1 6.4
1760 19.4 7.3
3439 23.5 14.5

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